Study of differences between sunspot area data determined from ground-based and space-borne observations

被引:5
|
作者
Györi, L
Baranyi, T
Turmon, M
Pap, JM
机构
[1] Heliophys Observ, Gyula Observing Stn, H-5701 Gyula, Hungary
[2] Heliophys Observ, H-4010 Debrecen, Hungary
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] Univ Maryland Baltimore Cty, Goddard Earth Sci & Technol Ctr, Greenbelt, MD USA
来源
SOLAR VARIABILITY AND CLIMATE CHANGE | 2004年 / 34卷 / 02期
基金
匈牙利科学研究基金会; 美国国家航空航天局;
关键词
sunspots; solar irradiance; sunspot area measurements; solarphysics;
D O I
10.1016/j.asr.2004.02.009
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The determination of the area of sunspots is important from several points of view, e.g, in study of the evolution of sunspots and their effect on solar irradiance. Automated sunspot area measurements are now replacing time-consuming and subjective hand-made measurements. Also, terrestrial solar observations have been supplemented by observations from space. The resolution of the ground observations is limited by the seeing, while space-borne observations are limited by the size of the CCD array. The use of different data sources, as well as of different region identification algorithms, causes discrepancies in reported sunspot areas. An important task is to determine to what extent these differences can be attributed to different analysis methods and to what extent to different data. It is also important to establish the required spatial resolution of space-based images. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:269 / 273
页数:5
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